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This Defense Intelligence Agency reference document, dated 11 March 2010, is one of the advanced technology reports produced in FY 2009 under the Advanced Aerospace Weapon System Applications (AAWSA) program. It introduces the Statistical Drake Equation, which replaces each factor of Frank Drake's 1961 equation with a uniform random variable to estimate how far away the nearest extraterrestrial civilization is. In the worked example, there is a 75% probability that the nearest civilization lies between 1,361 and 3,979 light years from Earth.
UNCLASSIFIED//F81it 8FFIIIAI!: 1!181! &••1::Y (26) where (25) wa~ already used in thc la~t stcp. By virtuc of the uniform prohahility density function ( 10) and of (26), the general tramformation law (9) finally yields b1 - a 1 (27) In other words, the requested pdf of Y, i~ i = I. .... 7 lm(a,)sy,ln(h,)I (28) Probability density functions of the natural logs of all the u11ifarmly di.~tributed Drake randam variable~· D, . This is indeed a positive function of.\· over the interval In(uJ :S: y :S: ln(hJ, as for every pdf, and it 1s casy lu sec thal its normaliLation cundition is fulfilled: ... (29) Next we want to find the mean value and standard deviation of Y, , since these play a crucial role for fulurc dcvclopmcnl~. The mean ialuc (Y,) i~ given by i ln(I> ) ( ) iln(I,, I v . e ,. (Y,)= 'v· f V dv= -·--d; ln(u,l • Y, - • ln(u,)b;-(1; • b, [In(b, )- I]- a, [1,;(u, )- I] b1 - 11, (30) This is thus the mean value of the nat11ral log of all the unifarmly di.~tributed Drake random variable.1· D, 36 In order to find the variance abo, we must first compute lhc mean value of the square of Y,, lhat is = h, [in 2 (h 1 )- 2 ln (h 1 )+ 2 ]- a, [tn 2 (a,)- 2 ln(a; )+ 2] h; -,1; ... (32) The variance of Y; = 1n(D;) is now given by (32) minus the square of (31 ), that. after a few reductions. yield: 2 a,h;[ln(h,)-ln(a,)] 2 =a,n(n,l=l- ( )' h, -a, Whence the corresponding standard deviation (34) Let us now turn to another topic: the use of fouricr tran~forms, that, in probahility theory, arc called ·'characteristic functions," following again the notations of Papoulis (ref [51) we call "'characteristic function", y_ (;) , of an assigned probability distribution Y1 , the Fourier transform of the relel'ant probability density function, that is (with j = μ) The use of characteristic function~ simplifies things greatly. For instance, the calculation of all moments of a known pdf becomes trivial if the relevant characteristic function is known, and greatly simplified also arc the proofs of important theorems of slalistics, like lhc Ccnlral Limit Theorem thal wc will use in Section 4. Anolhcr imporlanl rcsull i~ that thc characteristic function of lhc sum of a finitc numhcr of independent random variable~ is simply gi vcn by the product of the corresponding characteristic functions. This i~ just the case we arc facing in the Statistical Drake equation (3) and so we are now led to find the characteristic function of the random l'ariable Y1. i.e. UNCLASSIFIED//509 AEEIC:12 k !Pi'i ,ulklf
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Report, from the dia collection. The PDF is mirrored here; the original link is above. 55 pages are in the text index: search them above, or from the library's search.